4.4 Article

The MBTA pipeline for detecting compact binary coalescences in the third LIGO-Virgo observing run

Journal

CLASSICAL AND QUANTUM GRAVITY
Volume 38, Issue 9, Pages -

Publisher

IOP Publishing Ltd
DOI: 10.1088/1361-6382/abe913

Keywords

gravitational waves; astrophysics; data analysis techniques; general relativity; cosmology

Funding

  1. United States National Science Foundation (NSF)
  2. Australian Research Council
  3. European Gravitational Observatory (EGO)
  4. French Center National de Recherche Scientifique (CNRS)
  5. Italian Istituto Nazionale della Fisica Nucleare (INFN)
  6. Dutch Nikhef
  7. Science and Technology Facilities Council (STFC) of the United Kingdom
  8. Max-Planck-Society (MPS)
  9. State of Niedersachsen/Germany

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The study describes a method for searching gravitational wave signals in LIGO-Virgo data, including both real-time detection and offline analysis. The experimental results demonstrate that MBTA has a low median latency of 36 seconds and has contributed to 42 alerts.
We describe the multi-band template analysis (MBTA) search for gravitational waves signals from coalescences of compact objects in the LIGO-Virgo data, at the time of the third observing run (2019-2020), both for low-latency detections and for offline analysis. Details are given on the architecture and functioning of the pipeline, including transient noise mitigation strategies, parameter space for the searched signals, detection of candidates and evaluation of a false alarm rate associated to them. The performance of the low-latency search is demonstrated based on the LIGO-Virgo third observing run, during which MBTA has contributed to 42 alerts, submitting candidates with a median latency of 36 s. The performance of the offline search is illustrated on a subset of data collected during the second LIGO-Virgo observation run in 2017, and are quantified based on injections of simulated signal events on the same data.

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